Tuesday 15 September
Introduction and outline of the meeting
8:00 – 8:30 D. Elbaz, L. Spinoglio, T. Nagao and K. Kohno
Gaining the full 3D perspective on Star Formation and Black Hole accretion
[C. Gruppioni & G. Rodighiero]
8:30 – 9:00 Descoping the spectrophotometric surveys: a revision of the reference program. 9:00 – 9:45 Impact of the loss of SMI-CAM and SMI-LR ability to replace SMI-CAM for imaging.
9:45 – 10:00 Break
10:00 – 10:30 YB revision, figure updates.
Establishing the role of obscured BH-growth in the evolution of galaxies
[F. Pozzi, C. Vignali]
10:30 – 11:00 Synergies Athena/SPICA without SMI-CAM. What can be recovered using SMI-LR as an imager?
11:00 – 11:30 Yellow book updates, changes in figures.
11:30 – 11:45 Break
The origin and evolution of large-scale coherent magnetic fields in galaxies
11:45 – 12:10 Is a B-BOP polarimetric only survey useful/feasible? Possible implementation. 12:10 – 12:30 YB revision. Shall we group all polarization science in a separate section to strengthen the originality of this aspect of SPICA?
White papers, how are they affected by the descope?
12:30 – 13:00 L. Barchiesi, L. Bisigello, L. Ciesla, J.A. Fernández-Ontiveros, …